The number density of a charged relic
arXiv:0807.0211 · doi:10.1088/1475-7516/2008/10/005
Abstract
We investigate scenarios in which a charged, long-lived scalar particle decouples from the primordial plasma in the Early Universe. We compute the number density at time of freeze-out considering both the cases of abelian and non-abelian interactions and including the effect of Sommerfeld enhancement at low initial velocity. We also discuss as extreme case the maximal cross section that fulfils the unitarity bound. We then compare these number densities to the exotic nuclei searches for stable relics and to the BBN bounds on unstable relics and draw conclusions for the cases of a stau or stop NLSP in supersymmetric models with a gravitino or axino LSP.
45 pages
References in corpus (7)
- Full one-loop corrections to the relic density in the MSSM: A few examples
- Circumscribing Late Dark Matter Decays Model Independently
- Solving the cosmic lithium problems with primordial late-decaying particles
- Determining Reheating Temperature at Colliders with Axino or Gravitino Dark Matter
- SO(10) SUSY GUTs, the gravitino problem, non-thermal leptogenesis and axino dark matter
- Probing the Reheating Temperature at Colliders and with Primordial Nucleosynthesis
- Cascading to the MSSM